Fig. 7
Star-formation rate against hard X-ray luminosity for X-ray selected AGNs. We plot values of 99 far-infrared detected X-ray AGNs, and 32 FIR upper limits in the area covered by the deep Herschel survey. The dotted line is the expected FIR luminosity of a pure-AGN source, translated into SFR (see Mullaney et al. 2011). We find a strong correlation between the star-formation rate and the X-ray luminosity.
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